activity
20052009
most citedIntracluster Medium Entropy Profiles for a Chandra Archival Sample of Galaxy Clusters

571 citations · 1.6k across the 7 of their papers we have counts for

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6 papers · 1 filter

astro-ph200887 cited

Conduction and the Star-Formation Threshold in Brightest Cluster Galaxies

G. M. Voit, K. W. Cavagnolo, M. Donahue +3

Current models of galaxy evolution suggest that feedback from active galactic nuclei is needed to explain the high-luminosity cutoff in the galaxy luminosity function. Exactly how…

astro-ph2008249 cited

An Entropy Threshold for Strong H-alpha and Radio Emission in the Cores of Galaxy Clusters

Kenneth W. Cavagnolo, Megan Donahue, G. Mark Voit +1

Our Chandra X-ray Observatory archival study of intracluster entropy in a sample of 222 galaxy clusters shows that H-alpha and radio emission from the brightest cluster galaxy are…

astro-ph200859 cited

Bandpass Dependence of X-ray Temperatures in Galaxy Clusters

Kenneth W. Cavagnolo, Megan Donahue, G. Mark Voit +1

We explore the band dependence of the inferred X-ray temperature of the intracluster medium (ICM) for 192 well-observed galaxy clusters selected from the Chandra Data Archive. If t…

astro-ph200728 cited

Star Formation, Radio Sources, Cooling X-ray Gas, and Galaxy Interactions in the Brightest Cluster Galaxy in 2A0335+096

Megan Donahue, Ming Sun, Christopher P. O'Dea +2

We present deep emission-line imaging taken with the SOAR Optical Imaging Camera of the brightest cluster galaxy (BCG) in the nearby (z=0.035) X-ray cluster 2A0335+096. We analyze…

astro-ph20064 cited

Abundances of s-process elements in planetary nebulae: Br, Kr & Xe

Y. Zhang, R. Williams, E. Pellegrini +5

We identify emission lines of post-iron peak elements in very high signal-to-noise spectra of a sample of planetary nebulae. Analysis of lines from ions of Kr and Xe reveals enhanc…

astro-ph2005

Entropy Profiles in the Cores of Cooling Flow Clusters of Galaxies

Megan Donahue, Donald J. Horner, Kenneth W. Cavagnolo +1

The X-ray properties of a relaxed cluster of galaxies are determined primarily by its gravitational potential well and the entropy distribution of its intracluster gas. That entrop…